A dataset provided by the European Space Agency

Name 5384
Title RESOLVED AND COMPOSITE PROPERTIES OF THE GIANT HII REGIONS IN M33 CYCLE4MEDIUM
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=5384;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-fimztvk
Author Waller, William
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=5384&mission=hst
Publication
  • A 2D multiwavelength study of the ionized gas and stellar population in the giant H II region NGC 588
  • A Cepheid is No More: Hubbles Variable 19 in M33
  • Ages of M33 Star Clusters Based on the Hubble Space Telescope/WFPC2 Photometry
  • Blue Luminous Stars in Nearby Galaxies--UIT 005: A Possible Link to the Luminous Blue Variable Stage
  • Chandra ACIS Survey of M33 (ChASeM33): A First Look
  • Far-Ultraviolet Spectroscopy of Star-forming Regions in Nearby Galaxies: Stellar Populations and Abundance Indicators
  • Formation time-scales for high-mass X-ray binaries in M33
  • Interstellar H2 in M 33 detected with FUSE
  • Multiwavelength study of M33s giant HII regions NGC 588 and NGC 592
  • NGC 604, the Scaled OB Association (SOBA) Prototype. I. Spatial Distribution of the Different Gas Phases and Attenuation by Dust
  • On the importance of the few most massive stars: The ionizing cluster of NGC 588
  • Star cluster formation and disruption time-scales - I. An empirical determination of the disruption time of star clusters in four galaxies
  • Star Clusters in M33. I. Detection, Morphology, and Photometry
  • Star Clusters in M33. III. The Youngest Population
  • STIS Spectral Imagery of the OB Stars in NGC 604. II. The Most Luminous Stars
  • Structural Properties of Massive Young Clusters
  • The Discovery and Origin of a Very High-velocity Cloud Toward M33
  • The massive stellar content of the Hii region NGC 604 and its evolutionary state
  • The Stellar Initial Mass Function in the Giant HII Region NGC 595
  • The Very Faint End of the UV Luminosity Function over Cosmic Time: Constraints from the Local Group Fossil Record
  • Triggering the formation of the supergiant H II region NGC 604 in M 33
  • Unveiling the New Generation of Stars in NGC 604 with Gemini-NIRI
  • Wolf-Rayet stars in M33 - II. Optical spectroscopy of emission-line stars in giant HII regions
Instrument WFPC2, WFPC2/PC
Temporal Coverage 1994-06-19T18:44:17Z/1994-10-28T12:29:17Z
Version 1.0
Mission Description Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 1995-10-29T00:35:01Z
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Waller comma William, 1995, 'RESOLVED AND COMPOSITE PROPERTIES OF THE GIANT HII REGIONS IN M33 CYCLE4MEDIUM', 1.0, European Space Agency, https://doi.org/10.5270/esa-fimztvk